6533b86efe1ef96bd12cbeac

RESEARCH PRODUCT

Fitting Simpson's neutrino into the standard model

Jose W.f. Valle

subject

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsDirac (video compression format)Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFísicaStandard ModelGoldstone bosonMeasurements of neutrino speedHigh Energy Physics::ExperimentSymmetry breakingNeutrinoNeutrino oscillationParticle Physics - PhenomenologyLepton

description

Abstract I show how to accomodate the 17 keV state recently reported by Simpson as one of the neutrinos of the standard model. Experimental constraints can only be satisfied if the μ and τ neutrino combine to a very good approximation to form a Dirac neutrino of 17 keV leaving a light ν e . Neutrino oscillations will provide the most stringent test of the model. The cosmological bounds are also satisfied in a natural way in models with Goldstone bosons. Explicit examples are given in the framework of majoron-type models. Constraints on the lepton symmetry breaking scale which follow from astrophysics, cosmology and laboratory experiments are discussed.

10.1016/0370-2693(85)90118-2http://hdl.handle.net/10550/47209